Abstract
Line intensities of the two 12 C 16 O 2 laser bands ( ν 3– ν 1 and ν 3–2 ν 2 0) centered near 960.9 and 1063.7 cm −1 , respectively, were obtained from analysis of 30 room temperature long path laboratory absorption spectra recorded at 0.0028 and 0.0053 cm −1 resolution with the McMath–Pierce Fourier transform spectrometer at the National Solar Observatory (located on Kitt Peak). The spectra were analyzed simultaneously with the multispectrum nonlinear least-squares fitting procedure. The measured line intensities were further analyzed to derive the vibrational band intensities and Herman–Wallis coefficients.
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